'Radiation energy' presentation slideshows

Electromagnetic Spectrum and Laws of Radiation

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Radiation Parameterization

Radiation Parameterization. 2 November 2012. Thematic Outline of Basic Concepts. Why is radiation important? What are the fundamental processes that must be represented by a radiation parameterization? How are radiative transfer processes handled within a radiation parameterization?

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Chapter 3: Energy

Chapter 3: Energy. What are some types of energy?. Brainstorm about a type of energy as a group. Define this type of energy Where does it come from? How do we use it? What are some common examples?. Elastic Energy. Energy stored in an object due to its compression or extension.

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Radiation Heat Transfer

Radiation Heat Transfer. The Nature and Characteristics of Thermal Radiation. The Sun. Formed 49 x 10 9 years ago when a hydrogen molecular cloud collapsed rapidly Surface composition 92.0% H 2 7.0% He 1.0% Fe, Ni, O 2 . Si, S, Mg, C, Ne, Ca & Cr

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This work is licensed under a Creative Commons Attribution-Noncommercial-Share Alike 2.0 UK: England & Wales License

Basics on Molecular Spectroscopy. University of Lincoln presentation. This work is licensed under a Creative Commons Attribution-Noncommercial-Share Alike 2.0 UK: England & Wales License. SPECTROSCOPY. Interaction of Radiation with a sample

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Sun Protection

Sun Protection. Understanding the Danger. Why use sunscreen?. Too Much Sun Exposure is Bad for Your Body. Premature skin aging (wrinkles) Sunburns Skin cancer Cataracts. Sources: http://www.oasishospital.org/previousnews.html; http://wohba.com/archive/2005_03_01_archive.html.

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Ecology for Kids Vocabulary

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Stellar Evolution

Stellar Evolution. Chapter 12. Think, Pair, Share. Our sun started out as a: Protostar Class G star Neutron star Red giant star. Which stars are the most prevalent in the universe? Which are the least? How do stars sustain their fusion?

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FISICA AMBIENTALE 1

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Determination of coherent radiation spectra from interferograms

Determination of coherent radiation spectra from interferograms. Gennady Naumenko Tomsk Polytechnic University. Contents. Traditional interferometers Michelson interferometers Martin-Puplett interferometers Divided wave front (DWF) interferometer .

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Introduction to I njuries

Introduction to I njuries. Medico legal module 21 st batch June 2014. Dr Sanjaya Hulathduwa MBBS , MD, DLM, DMJ Path( Lond ) DMJ Clin ( Lond ) , Dip. Crim MFFLM(UK) Senior Lecturer.

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Radiation Units

Radiation Units. 1-Radioactivity Units. Physical Units Becquerel Amount of radioactive sample s.t. there is 1 atomic decay per second Henri Becquerel: discovered radioactivity through experiments with uranium and other radioactive matter Curie (Ci) 3.7*10 10 decays per second

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Radiation Protection Procedures

Radiation Protection Procedures. Chapters 39-40 Bushong Chapter 1 Sherer. Units of measurement. Exposure -Radiation intensity of air What is the unit of measurement? Dose-radiation energy absorbed from radiation exposure What is the unit of measurement?

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More about ? , ? and ? Radiation

More about ? , ? and ? Radiation. Nuclear Physics Lesson 3. Homework. Find out how they determined the nature of ? , ? and ? radiation. Learning Objectives. Recall what is meant by the term ionisation. Derive the inverse square law. Recall the equations for radioactive change.

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Nuclear Energy

Nuclear Energy. Nuclear Reactions - when unstable isotopes gain stability by making changes in the nucleus. These changes are followed by large amounts of radiation energy. Radioisotopes -isotopes that have unstable nuclei. *Stability depends on ratio of neutrons to protons.

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Radiation (Ch 12 YAC)

Radiation (Ch 12 YAC).

154 views • 9 slides